电子移相方法的讨论

对精密测试中常用的几种移相方法进行了讨论,主要浅析小角度电路移相方法。     

飞秒激光激励闪锌矿晶体产生太赫兹辐射的数学分析

基于飞秒激光激励闪锌矿晶体的太赫兹源实现方法较为简单,已有研究证明发射效率与晶体晶向选择,飞秒激光入射角以及偏振态相关,文章通过详细的理论分析与数学计算,讨论了正入射以及斜入射情况下太赫兹辐射最优化条件,获得了明确的飞秒激光入射角、偏振态、晶体晶向的选择依据,对提高太赫兹输出效率具有重要的指导意义。     

Detection of aerosol pollution sources during sandstorms in Northwestern China using remote sensed and model simulated data

The present paper has used a comprehensive approach to study atmosphere pollution sources including the study of vertical distribution characteristics, the epicenters of occurrence and transport of atmospheric aerosol in North-West China under intensive dust storm registered in all cities of the region in April 2014. To achieve this goal, the remote sensing data using Moderate Resolution Imaging Spectroradiometer satellite (MODIS) as well as model-simulated data, were used, which facilitate tracking the sources, routes, and spatial extent of dust storms. The results of the study have shown strong territory pollution with aerosol during sandstorm. According to ground-based air quality monitoring stations data, concentrations of PM₁₀ and PM_2.5 exceeded 400?μg/m³ and 150?μg/m³, respectively, the ratio PM_2.5/PM₁₀ being within the range of 0.123–0.661. According to MODIS/Terra Collection 6 Level-2 aerosol products data and the Deep Blue algorithm data, the aerosol optical depth (AOD) at 550?nm in the pollution epicenter was within 0.75–1. The vertical distribution of aerosols indicates that the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO) 532?nm total attenuates backscatter coefficient ranges from 0.01 to 0.0001?km^?1?×?sr^?1 with the distribution of the main types of aerosols in the troposphere of the region within 0–12.5?km, where the most severe aerosol contamination is observed in the lower troposphere (at 3–6?km). According to satellite sounding and model-simulated data, the sources of pollution are the deserted regions of Northern and Northwestern China.     

Three dimensional temperature field in a conducting sphere due to an arbitrarily located split ring heating source

Thermal control of spacecrafts plays an important role in space missions. In the design stage the preliminary thermal analysis of the spacecraft requires an estimate of the conductive thermal resistance between the various spacecraft components. With this in mind, the fully three dimensional problem of determining the thermal field in a conducting sphere with an asymmetric split ring current carrying heating source is resolved in an analytical or almost analytical form, implying either a closed form solution or utmost expressions involving a simple numerical integration. This has immediate application for evaluation of thermal resistance in spacecrafts. Green's function integral techniques are used. Comparisons are made with series solutions and also with purely numerical solutions to contrast the simplicity and highlight the elegance of the present method. Parametric studies reveal expected behavior.     

Assessment of precision in ionospheric electron density profiles retrieved by GPS radio occultations

The Constellation Observing System for Meteorology Ionosphere and Climate (COSMIC) is a six satellite radio occultation mission that was launched in April 2006. The close proximity of these satellites during some months after launch provides a unique opportunity to evaluate the precision of Global Positioning System (GPS) radio occultation (RO) retrievals of ionospheric electron density from nearly collocated and simultaneous observations. RO data from 30 consecutive days during July and August 2006 are divided into ten groups in terms of daytime or nighttime and latitude. In all cases, the best precision values (about 1%) are found at the F peak height and they slightly degrade upwards. For all daytime groups, it is seen that electron density profiles above about 120 km height exhibit a substantial improvement in precision. Nighttime groups are rather diverse: in particular, the precision becomes better than 10% above different levels between 120 and 200 km height. Our overall results show that up to 100–200 km (depending on each group), the uncertainty associated with the precision is in the order of the measured electron density values. Even worse, the retrieved values tend sometimes to be negative. Although we cannot rely directly on electron density values at these altitudes, the shape of the profiles could be indicative of some ionospheric features (e.g. waves and sporadic E layers). Above 200 km, the profiles of precision are qualitatively quite independent from daytime or latitude. From all the nearly collocated pairs studied, only 49 exhibited a difference between line of sight angles of both RO at the F peak height larger than 10°. After analyzing them we find no clear indications of a significant representativeness error in electron density profiles due to the spherical assumption above 120 km height. Differences in precision between setting and rising GPS RO may be attributed to the modification of the processing algorithms applied to rising cases during the initial period of the COSMIC mission.     

光电自准直仪自适应光源设计方法研究

介绍了一种自适应光源设计方法。利用反馈原理自动校正自准直光源参数,调节发光强度,降低了自准直仪对反光面、使用环境的苛刻要求,提高了仪器的环境通用性及测量精度。     

基于分布式信源编码和感兴趣区域编码的干涉多光谱图像压缩

基于干涉多光谱图像特点和应用环境要求,提出一种基于分布式信源编码和感兴趣区域编码的干涉多光谱图像压缩算法。编码端通过关键帧预测出边信息帧,然后联合估计的边信息帧和插值分布的概率模型在编码端进行比特平面码率估计,最后采用基于率失真提升的感兴趣区域编码,调整图像不同区域的率失真斜率来进行更合理的码率分配。实验结果表明,该算法比传统算法更好地保护了多光谱图像的光谱信息。在不同压缩比的情况下,这种编码方式在干涉多光谱图像压缩系统中可获得较好的效果,算法复杂度低。     

HOTDISK在低导热材料测试中的重复性分析

HOTDISK在工程材料导热系数测试中有着广泛应用。通过用HOTDISK对气凝胶粉体、保温毯和保温绝热板的测试,对比了不同时间段测试结果的波动情况,根据数据波动规律给出了测试过程中需要注意的事项和相应的改进建议。     

用于火星探测的电子分析器定标

用于火星探测的电子分析器采用了带偏转板的同轴圆柱形静电分析器, 该传感器方案在满足性能指标的同时实现了小型化. 利用法国空间辐射研究中心(CESR)的电子源, 对电子分析器两个传感器通道的静电分析器因子、能量分辨率、偏转板偏转因子、 方位角分辨率和极角分辨率进行了定标. 给出了上述参数的定标结果, 并对结果进行了分析. 结果表明,仪器的能量范围、能量分辨率、方位角视场及角度分辨率等参数均优于指标要求. 定标结果为电子分析器在轨数据处理和分析以及在轨运行参数设置提供了依据.